PMO OpenIR  > 太阳活动的多波段观测研究团组
Time evolution of the turnover frequency for diagnosis of the coronal magnetic field
Huang, GL
2006
Source PublicationCHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
ISSN1009-9271
Volume6Issue:1Pages:113-119
AbstractTwo impulsive microwave bursts observed by Owens-Valley Solar Arrays (OVSA) are studied. The fast time variation of the turnover frequency in these bursts is quite different from the constant value in the earlier conclusion. The observational turnover frequencies are consistent with the calculations using the non-thermal gyrosynchrotron radiation model. We find the turnover frequency may play an important role for calculating the coronal magnetic field on the basis of Dulk and Marsh's approximations.
KeywordSun : Radio Radiation Sun : Corona Sun : Magnetic Fields
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordSOLAR MICROWAVE-BURSTS ; NONTHERMAL ELECTRONS ; RADIO-EMISSION
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000235501700012
Citation statistics
Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/3506
Collection太阳活动的多波段观测研究团组
AffiliationChinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
Recommended Citation
GB/T 7714
Huang, GL. Time evolution of the turnover frequency for diagnosis of the coronal magnetic field[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2006,6(1):113-119.
APA Huang, GL.(2006).Time evolution of the turnover frequency for diagnosis of the coronal magnetic field.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,6(1),113-119.
MLA Huang, GL."Time evolution of the turnover frequency for diagnosis of the coronal magnetic field".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 6.1(2006):113-119.
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